HIP 2409
HIP 2409 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 2,051 light-years, HIP 2409 is a distant star lying deep within the Milky Way galaxy.
HIP 2409 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 2409 has an apparent magnitude of +7.39, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its blue hue, which corresponds to a B-V color index of -0.013.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.013 |
Observation
| Apparent Magnitude | +7.39 |
| Absolute Magnitude | -1.60 |
| Distance | 2,051 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 0h 30.69m |
| Declination | 62° 21.24′ |
Frequently Asked Questions
What type of star is HIP 2409?
HIP 2409 is a Class B — B-type (Blue-White) star.
How far is HIP 2409 from Earth?
HIP 2409 is approximately 2,051.3 light-years from Earth.
Can you see HIP 2409 with the naked eye?
With an apparent magnitude of 7.39, HIP 2409 is not visible to the naked eye.
What constellation is HIP 2409 in?
HIP 2409 is located in the constellation Cassiopeia.